In　the　background　of　a　charged　anti-de　Sitter　(AdS)　dilaton　black　hole,　we　investigate　the　movement　of　a　self-graviting　three-brane　and　relevant　holographic　effects　as　the　brane　moves　close　to　the　AdS　boundary.　The　induced　metric　on　the　brane　corresponds　to　an　exact　Friedmann-Lemaitre-Robertson-Walker　(FLRW)　geometry,　while　the　evolution　of　brane　is　determined　by　the　Israel　junction　condition　and　the　effective　Einstein　field　equation　on　the　brane　together.　When　the　brane　approaches　the　AdS　boundary,　AdS=CFT　correspondence　implies　that　a　radiation　dominated　FLRW　universe　(P　=　1/3　rho)　should　be　given.　According　to　the　holographic　renormalization　procedure,　we　involve　an　appropriate　surface　counterterm　into　the　gravitational　action　for　achieving　P　=　1/3　rho　on　the　brane.　This　surface　counterterm　also　plays　an　important　role　in　calculating　the　mass　of　a　charged　AdS　dilaton　black　hole.　Finally,　we　obtain　the　thermodynamic　quantities　and　give　an　extended　Cardy-Verlinde　formula　on　the　brane.